Summary
CoRoT-16b is a transiting exoplanet orbiting the G or K type main sequence star CoRoT-16 2,433 light years[4] away in the southern constellation Scutum. The planet was discovered in June 2011 by the French-led CoRoT mission.
 CoRoT-16 compared to Jupiter | |
| Discovery[1] | |
|---|---|
| Discovered by | Ollivier et al. |
| Discovery site | CoRoT space telescope |
| Discovery date | 10 June 2011 |
| Transit | |
| Orbital characteristics | |
| Apastron | 0.0847 AU (12,670,000 km) |
| Periastron | 0.0389 AU (5,820,000 km) |
| 0.0618 ± 0.0015 AU (9,250,000 ± 220,000 km)[1] | |
| Eccentricity | 0.37+0.11 −0.12[2] |
| 5.35227±0.00020 d[1] | |
| Inclination | 85.01°+0.94° −1.20°[1] |
| 2,454,923.9145±0.0022 JD[2] | |
| 161°+33° −29°[2] | |
| Semi-amplitude | 62.6+11.0 −9.9 km/s[2] |
| Star | CoRoT-16 |
| Physical characteristics | |
Mean radius | 1.17+0.14 −0.16 RJ[2] |
| Mass | 0.529+0.098 −0.096 MJ[2] |
Mean density | 0.41+0.22 −0.14 g/cm3[2] |
| Temperature | 1,086 K (813 °C; 1,495 °F)[3] |
Discovery edit
CoRoT-16b was detected using the transit method, which measures the brightness changes during an eclipse. However, this planet has an eccentric orbit, which is unusual due to CoRoT-16b's proximity to its parent star and the age.[1]
Properties edit
Due to its orbit, CoRoT-16b is classified as a "hot Jupiter". It only takes about 5 days to orbit CoRoT-16, but has an unusually eccentric orbit. CoRoT-16b has 52.9% the mass of Jupiter, but is 17% larger than the latter. Due to the low mass and high radius, CoRoT-16b has 41% the density of water; the orbit gives it an equilibrium temperature of 1,086 K. However, this is only an estimate due to the eccentricity of CoRoT-16b.
References edit
- ^ a b c d e Ollivier, M.; et al. (May 2012). "Transiting exoplanets from the CoRoT space mission. XXII. CoRoT-16b: a hot Jupiter with a hint of eccentricity around a faint solar-like star". Astronomy and Astrophysics. 541: A149. Bibcode:2012A&A...541A.149O. doi:10.1051/0004-6361/201117460. ISSN 0004-6361.
- ^ a b c d e f g Bonomo, A. S.; et al. (1 June 2017). "The GAPS Programme with HARPS-N at TNG . XIV. Investigating giant planet migration history via improved eccentricity and mass determination for 231 transiting planets". Astronomy and Astrophysics. 602: A107. arXiv:1704.00373. Bibcode:2017A&A...602A.107B. doi:10.1051/0004-6361/201629882. ISSN 0004-6361.
- ^ "Open Exoplanet Catalogue - CoRoT-16b". Open Exoplanet Catalogue. Retrieved 24 November 2021.
- ^ Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv:1804.09365. Bibcode:2018A&A...616A...1G. doi:10.1051/0004-6361/201833051. Gaia DR2 record for this source at VizieR.